SPECTROGRAPHY, August 2006


Date : August 2006

Location : Pises Observatory

Intrument : Intes 180mm + Modified Losmandy G-11 (optique et vision)

Guiding camera : Vesta pro

Imaging camera : SBIG ST7

Tracking system : MCMT II

Spectrograph : Lhires III, using 2400 lines per mm grating, slit width estimated to 25 to 30 µm (3").

The acquisition and tracking was achieved using PRISM v6 software, as well the spectra were all processed and calibrated using this software.See here (PRISM's newletters). All spectra are made of 60s single exposures

The observers (P.Roblin and myself)

ARCTURUS

This is a K1 type star (redhish an rather old), this the spectra from 652 nm to 661 nm, Halpha is absorbed (1260s exposure time).

 

ALTAIR

A7V blue star, showing a wide halpha absorption band (Only 120s).

Here due to failure from neon lamp, spectral calibration was not performed. Atmospheric lines can be used instead.

P-CYGNI

This is a peculiar B star, with an absorption line nearby a strong Halpha line (5000sec).

 

BSC8297 (Cygni) said as "RV Cyg"

This is a mag 6 C6 type star, it has a deep red color and is an old star, called as carbon stars. B-V magnitude index is 2.5 !

The spectra is pretty unusual !! Very convenient for testing spectrograph resolution (1300s exposure time).

Here due to failure from neon lamp (camera alignement was also changed), spectral calibration was not performed.

Gamma CAS

Gamma Cassiopea is a famous BE star, Mag 2.47 featuring a strong H-alpha emission line that changes over the time. 2800s exposure

BSC 8146 (Cygni)

This a magnitude 4.43 Be Star (600s exposure time)

Here due to failure from neon lamp, spectral calibration was not performed. Atmospheric lines can be used instead.

DELTA CASS

A mag2.7 A5 type star, a spectra very close to Altair, 1900s exposure time.

64 Cygni

This is a G8 star, magnitude 3.2. 600s exposure time. As a G8 star, this one is very close to the SUN physicaly speaking (more or less same spectra lines)

Here (again) due to failure from neon lamp, spectral calibration was not performed. Atmospheric lines can be used instead.

CYGNI stars map


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